Disk masses used in different theoretical planetary population synthesis works. Shaded regions or error bars show the 1σ scatter in the distributions. Log-uniform distributions are used to sample disk masses in all works except for Miguel et al. (2020) who draw from a linear-uniform distribution (1 × 10⁻⁴ M_⊙ to 5 × 10⁻² M_⊙). They are also the only work which samples over stellar masses instead of using fixed values. Liu et al. (2020) prescribe stellar accretion rates as opposed to disk masses; the data shown here corresponds to integrating from time zero to 10 Myr. The “heavy disk” case of Alibert & Benz (2017, open-circle, scatter-omitted) draws disks with twice their nominal mass. Apart from this case, we show the distributions labeled as nominal by the respective authors. The disk masses used in this work are in agreement to previous assumptions.